Energetic Particle Physics in Tokamak Plasmas Guoyong Fu Princeton Plasma Physics Laboratory Princeton University Princeton, NJ 08543, USA 6 th Workshop.
Judy Karpen, Spiro Antiochos, Rick DeVore, and Mark Linton MHD Simulations of Flux Cancellation on the Sun* *Work supported by ONR and NASA.
How Does Free Magnetic Energy Enter the Corona? Brian Welsch, Space Sciences Lab, UC Berkeley Free magnetic energy, equivalent to departures of the coronal.
How Does Free Magnetic Energy Enter the Corona?
Students, introduce yourselves: where from, what year, main interests.
Relaxation of Sheared Magnetic fields — a Process of Contraction
Turbulent transport in collisionless plasmas: eddy mixing or wave-particle decorrelation? Z. Lin Y. Nishimura, I. Holod, W. L. Zhang, Y. Xiao, L. Chen.
Introduction to Gyrokinetic Theory & Simulations Greg Hammett (Princeton University, PPPL) ITER Summer School, Aix-en-Provence, Aug. 26, 2014 (these slides.
Graham Steward 1, Vasily Lobzin 1, Mike Terkildsen 1, Matt Francis 1, Iver Cairns 2 (1) Bureau of Meteorology, Space Weather Services, Sydney, Australia;
Overview of Neutron and Escaping Alpha Diagnostics Planned for ITER
Turbulent transport in collisionless plasmas: eddy mixing or wave-particle decorrelation? Z. Lin
Patterns of Large-Scale Flux Emegence
